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Transcript
Chapter 25
Reflection and Refraction
of Light
Fig. 25-CO,2p. 839
25.1 The Nature of Light


Before the beginning of the nineteenth
century, light was considered to be a stream
of particles
The particles were emitted by the object
being viewed,


Newton was the chief architect of the particle
theory of light
He believed the particles left the object and
stimulated the sense of sight upon entering the
eyes
3
Nature of Light –
Alternative View


Christian Huygens argued the light
might be some sort of a wave motion
Thomas Young (1801) provided the first
clear demonstration of the wave nature
of light


He showed that light rays interfere with
each other
Such behavior could not be explained by
particles
4
More Confirmation
of Wave Nature



During the nineteenth century, other
developments led to the general
acceptance of the wave theory of light
Maxwell asserted that light was a form
of high-frequency electromagnetic wave
Hertz confirmed Maxwell’s predictions
5
Particle Nature


Some experiments could not be
explained by the wave nature of light
The photoelectric effect was a major
phenomenon not explained by waves


When light strikes a metal surface,
electrons are sometimes ejected from the
surface
The kinetic energy of the ejected electron
is independent of the frequency of the light
6
Dual Nature of Light


In view of these developments, light
must be regarded as having a dual
nature
In some cases, light acts like a wave,
and in others, it acts like a particle
7
The Ray Approximation
in Geometric Optics



Geometric optics involves the study of the
propagation of light
The ray approximation is used to represent
beams of light
A ray is a straight line drawn along the
direction of propagation of a single wave


It shows the path of the wave as it travels through
space
It is a simplification model
8
Ray Approximation


The rays are straight lines
perpendicular to the wave
fronts
With the ray approximation,
we assume that a wave
moving through a medium
travels in a straight line in
the direction of its rays
Fig 25.1
9
Ray Approximation
at a Barrier

A wave meets a barrier with
l<<d




d is the diameter of the opening
The individual waves
emerging from the opening
continue to move in a straight
line
This is the assumption of the
ray approximation
Good for the study of mirrors,
lenses, prisms, and
associated optical instruments
Fig 25.2(a)
10
Ray Approximation
at a Barrier, cont


The wave meets a
barrier whose size of the
opening is on the order
of the wavelength, l~d
The waves spread out
from the opening in all
directions

The waves undergo
diffraction
Fig 25.2(b)
11
Ray Approximation
at a Barrier, final

The wave meets a
barrier whose size of the
opening is much smaller
than the wavelength


l >> d
The diffraction is so
great that the opening
can be approximated as
a point source
Fig 25.2(c)
12
Active Figure
25.2
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13
Reflection of Light


A ray of light, the incident ray, travels in
a medium
When it encounters a boundary with a
second medium, part of the incident ray
is reflected back into the first medium

This means it is directed backward into the
first medium
14
Specular
Reflection



Specular reflection is
reflection from a smooth
surface
The reflected rays are
parallel to each other
All reflection in your text
is assumed to be
specular
Fig 25.4(a)
15
Diffuse
Reflection



Diffuse reflection is
reflection from a rough
surface
The reflected rays travel
in a variety of directions
A surface behaves as a
smooth surface as long
as the surface variations
are much smaller than
the wavelength of the
light
Fig 25.4(b)
16
Law of Reflection

The normal is a line
perpendicular to the surface



It is at the point where the
incident ray strikes the surface
The incident ray makes an
angle of θ1 with the normal
The reflected ray makes an
angle of θ1' with the normal
Fig 25.5
17
Active Figure
25.5
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18
Law of Reflection, cont


The angle of reflection is equal to the
angle of incidence
θ1'= θ1


This relationship is called the Law of
Reflection
The incident ray, the reflected ray and
the normal are all in the same plane
19
20p. 844
Fig. 25-6a,
21p. 844
Fig. 25-6b,
Multiple Reflections




The incident ray strikes the
first mirror
The reflected ray is directed
toward the second mirror
There is a second reflection
from the second mirror
Apply the Law of Reflection
and some geometry to
determine information about
the rays
Fig 25.7
22
Some Additional Points

The path of a light ray is reversible


This property is useful for geometric
constructions
Applications of the Law of Reflection
include digital projection of movies, TV
shows and computer presentations

Using a digital micromirror device

Contains more than a million tiny mirrors that
can be individually tilted and each corresponds
to a pixel in the image
23
24
25
26
25.4 Refraction of Light


When a ray of light traveling through a
transparent medium encounters a boundary
leading into another transparent medium, part
of the energy is reflected and part enters the
second medium
The ray that enters the second medium is
bent at the boundary

This bending of the ray is called refraction
27
Refraction, 2


The incident ray, the reflected ray, the
refracted ray, and the normal all lie on the
same plane
The angle of refraction depends upon the
material and the angle of incidence
sin 1 v 2

 constant
sin 2 v1

v1 is the speed of the light in the first medium and
v2 is its speed in the second medium
28
Refraction of Light, 3

The path of the light
through the refracting
surface is reversible


For example, a ray travels
from A to B
If the ray originated at B,
it would follow the line AB
to reach point A
Fig 25.8
29
Following the Reflected
and Refracted Rays





Ray  is the incident ray
Ray  is the reflected ray
Ray  is refracted into the
lucite
Ray  is internally reflected
in the lucite
Ray  is refracted as it
enters the air from the lucite
Fig 25.8
30
Active Figure
25.8
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31
25.4 Refraction Details, 1


Light may refract into a
material where its
speed is lower
The angle of refraction
is less than the angle of
incidence

The ray bends toward
the normal
Fig 25.9
32
Refraction Details, 2


Light may refract into a
material where its
speed is higher
The angle of refraction
is greater than the angle
of incidence

The ray bends away from
the normal
Fig 25.9
33
Active Figure
25.9
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34
Light in a Medium





The light enters from the left
The light may encounter an
atom, as in A
The atom may absorb the light,
oscillate, and reradiate the light
This can repeat at atom B
The absorption and radiation
cause the average speed of the
light moving through the
material to decrease
Fig 25.10
35
The Index of Refraction
The speed of light is a maximum in a
vacuum
 The index of refraction, n, of a medium
can be defined as
speed of light in a vacuum
n
average speed of light in a medium

c
n
v
36
Index of Refraction, cont

For a vacuum, n = 1



We assume n = 1 for air, also
For other media, n > 1
n is a dimensionless number greater
than unity

n is not necessarily an integer
37
Some Indices of Refraction
38
Frequency Between Media

As light travels from one
medium to another, its
frequency does not change


Both the wave speed and the
wavelength do change
The wavefronts do not pile up,
nor are created or destroyed at
the boundary, so ƒ must stay
the same
Fig 25.11
39
Index of Refraction Extended


The frequency stays the same as the wave
travels from one medium to the other
v=ƒλ


ƒ1 = ƒ2 but v1 v2 so l1 l2
The ratio of the indices of refraction of the two
media can be expressed as various ratios
c
l1 v1
n1 n2



l2 v 2 c
n1
n2
40
More About
Index of Refraction


The previous relationship can be
simplified to compare wavelengths and
indices: l1 n1 = l2 n2
In air, n1 1 and the index of refraction
of the material can be defined in terms
of the wavelengths
l  l in vacuum 
n


ln  l in material 
41
Snell’s Law of Refraction

n1 sin θ1 = n2 sin θ2



θ1 is the angle of incidence
θ2 is the angle of refraction
The experimental discovery of this
relationship is usually credited to
Willebrord Snell and therefore known as
Snell’s Law
42
25.5 Dispersion



For a given material, the index of
refraction varies with the wavelength of
the light passing through the material
This dependence of n on λ is called
dispersion
Snell’s Law indicates light of different
wavelengths is bent at different angles
when incident on a refracting material
43
44
45
46
47
48
49
50
51
52
53
Variation of Index of
Refraction with Wavelength


The index of refraction
for a material generally
decreases with
increasing wavelength
Violet light bends more
than red light when
passing into a refracting
material
Fig 25.13
54
Angle of Deviation


The ray emerges
refracted from its
original direction of
travel by an angle d,
called the angle of
deviation
d depends on F and
the index of
refraction of the
material
Fig 25.14
55
Refraction in a Prism

Since all the colors
have different
angles of deviation,
white light will
spread out into a
spectrum



Violet deviates the
most
Red deviates the least
The remaining colors
are in between
Fig 25.15
56
The Rainbow


A ray of light strikes a drop of water in
the atmosphere
It undergoes both reflection and
refraction

First refraction at the front of the drop


Violet light will deviate the most
Red light will deviate the least
57
The Rainbow, 2



At the back surface the light
is reflected
It is refracted again as it
returns to the front surface
and moves into the air
The rays leave the drop at
various angles


The angle between the white
light and the most intense
violet ray is 40°
The angle between the white
light and the most intense red
ray is 42°
Fig 25.16
58
Active Figure
25.16
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59
25.6 Observing the Rainbow



Fig 25.17
If a raindrop high in the sky is observed, the red ray is
seen
A drop lower in the sky would direct violet light to the
observer
The other colors of the spectra lie in between the red
and the violet
60
Double Rainbow



The secondary rainbow is
fainter than the primary and
its colors are reversed
The secondary rainbow
arises from light that makes
two reflections from the
interior surface before
exiting the raindrop
Higher-order rainbows are
possible, but their intensity is
low
61
Christiaan Huygens



1629 – 1695
Best known for his
contributions to the
fields of optics and
dynamics
He considered light to
be a kind of vibratory
motion, spreading out
and producing the
sensation of sight when
impinging on the eye
62
Huygen’s Principle


Huygen assumed that light consists of
waves rather than a stream of particles
Huygen’s Principle is a geometric
construction for determining the position
of a new wave at some point based on
the knowledge of the wave front that
preceded it
63
Huygen’s Principle, cont


All points on a given wave front are
taken as point sources for the
production of spherical secondary
waves, called wavelets, which
propagate outward through a medium
with speeds characteristic of waves in
that medium
After some time has passed, the new
position of the wave front is the
surface tangent to the wavelets
64
Huygen’s Construction
for a Plane Wave



At t = 0, the wave front is
indicated by the plane AA’
The points are
representative sources for
the wavelets
After the wavelets have
moved a distance cΔt, a new
plane BB’ can be drawn
tangent to the wavefronts

BB’ is parallel to AA’
Fig 25.18
65
Huygen’s Construction
for a Spherical Wave



The inner arc represents
part of the spherical
wave
The points are
representative points
where wavelets are
propagated
The new wavefront is
tangent at each point to
the wavelet
Fig 25.18
66
Huygen’s Principle, Example



Waves are generated in a
ripple tank
Plane waves produced to
the left of the slits emerge to
the right of the slits as twodimensional circular waves
propagating outward
At a later time, the tangent of
the circular waves remains a
straight line
Fig 25.19
67
Huygen’s Principle
and the Law of Reflection


The Law of Reflection
can be derived from
Huygen’s Principle
AB is a wave front of
incident light



The wave at A sends
out a wavelet centered
on A toward D
The wave at B sends
out a wavelet centered
on B toward C
AD = BC = c Dt
Fig 25.20
68
Huygen’s Principle and the
Law of Reflection, cont






Triangle ABC is
congruent to triangle
ADC
cos g = BC / AC
cos g’ = AD / AC
Therefore, cos g = cos g’
and gg’
This gives θ1 = θ1’
This is the Law of
Reflection
Fig 25.20
69
Huygen’s Principle
and the Law of Refraction


Ray 1 strikes the
surface and at a
time interval Dt later,
ray 2 strikes the
surface
During this time
interval, the wave at
A sends out a
wavelet, centered at
A, toward D
Fig 25.21
70
Huygen’s Principle and the
Law of Refraction, cont



The wave at B sends out a wavelet,
centered at B, toward C
The two wavelets travel in different
media, therefore their radii are different
From triangles ABC and ADC, we find
BC v1Dt
sin1 

AC AC
and
AD v 2 Dt
sin 2 

AC AC
71
Huygen’s Principle and the
Law of Refraction, final

The preceding equation can be simplified
to
sin1 v1

sin 2 v 2
sin1 c n1 n2
But


sin 2 c n2 n1
and so n1 sin1  n2 sin 2

This is Snell’s Law of Refraction
72
73
74
75
76
77
78
25.7 Total Internal Reflection

A phenomenon called total internal
reflection can occur when light is
directed from a medium having a given
index of refraction toward one having a
lower index of refraction
79
Possible Beam Directions


Possible directions
of the beam are
indicated by rays
numbered 1 through
5
The refracted rays
are bent away from
the normal since n1
> n2
Fig 25.22
80
Critical Angle

There is a particular
angle of incidence
that will result in an
angle of refraction of
90°

This angle of
incidence is called
the critical angle, C
sinC 
n2
for n1  n2
n1
Fig 25.22
81
Active Figure
25.22
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82
Critical Angle, cont

For angles of incidence greater than the
critical angle, the beam is entirely
reflected at the boundary


This ray obeys the Law of Reflection at the
boundary
Total internal reflection occurs only
when light is directed from a medium of
a given index of refraction toward a
medium of lower index of refraction
83
84
85
86
87
25.8 Optical Fibers



An application of
internal reflection
Plastic or glass rods are
used to “pipe” light from
one place to another
Applications include


medical use of fiber optic
cables for diagnosis and
correction of medical
problems
Telecommunications
Fig 25.25
88
Optical Fibers, cont


A flexible light pipe
is called an optical
fiber
A bundle of parallel
fibers (shown) can
be used to construct
an optical
transmission line
89
Construction
of an Optical Fiber

The transparent
core is surrounded
by cladding



The cladding has a lower
n than the core
This allows the light in
the core to experience
total internal reflection
The combination is
surrounded by the
jacket
Fig 25.26
90
Multimode,
Stepped Index Fiber


Stepped index
comes from the
discontinuity in n
between the core
and the cladding
Multimode means
that light entering
the fiber at many
angles is transmitted
Fig 25.27
91
Multimode,
Graded Index Fiber


This fiber has a core
whose index of
refraction is smaller
at larger radii from
the center
The resultant
curving reduces
transit time and
reduces spreading
out of the pulse
Fig 25.29
92
Optical Fibers, final



Optical fibers can transmit about 95% of
the input energy over one kilometer
Minimization of problems includes using
as long a wavelength as possible
Much optical fiber communication uses
wavelengths of about 1 300 nm.
93
94p. 857
Fig. 25-30,